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Journal of Physics A Mathematical and General

A model of cavity radiation with anti-bunched and sub-Poissonian characteristics

S. K. Srinivasan

Published Jul 11, 1986• 6 citations
Publisher

Abstract

The author proposes a model of cavity population in which each emission gives rise to a random dead time during which no further emissions are possible. The photon population statistics are shown to possess an anti-bunching character for an appropriate choice of parameters.
DOI
10.1088/0305-4470/19/10/007

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A detailed analysis is provided of a non-Markov model of cavity population in which each emission gives rise to a random dead-time during which no further emissions can take place. Differential equations are derived for the generating functions governing the cavity population size. The moment structure of the population size is examined and explicit expressions for the first two moments are provided. The photon population statistics are shown to be antibunched for a wide choice of the population parameters. The detection process is analysed and an explicit expression is provided for the Hanbury Brown-Twiss type of correlation. It is further shown that an appropriate choice of the population parameters can produce a thermal stream with Lorentzian profile.
A great deal of effort has been devoted during the last decade to the theory of nonclassical states of the radiation field. From a practical point of view some of the most interesting predictions of these theories concern the generation of light with sub-Poissonian photon counting statistics for which Such light is evidently less noisy than laser radiation with obvious implications for the improved performance of optical systems. When the temporal autocorrelation function of the photon counts increases as the delay time increases from zero the light is also said to be antibunched.
The population model of cavity photons previously introduced is analysed by identifying the non-Markov evolution in terms of phases whose durations are themselves independent and exponentially distributed random variables. The resulting radiation is shown to have thermal characteristics for an appropriate choice of the population parameters. The detection process is explicitly introduced and its characteristics are obtained. The model is shown to be viable enough to produce intensity spectra of different shapes corresponding to the resulting radiation.
Some of the implications of non-Markov evolution of cavity radiation and its detection are examined. The cavity photons are modelled as members of a population governed by a Bellman-Harris process supported by immigration. Further it is assumed that there is a detector near the cavity and the photosensitive atoms of the detector absorb the photons with a uniform probability η per unit time. Explicit expressions for the first two moments of the equilibrium cavity distribution are provided. A general formula for the spectral profile is also given. The Markov model of Shepherd is recovered as a special case. A detailed analysis is provided for a special case in which the photon is assumed to go through two hypothetical phases before it gives rise to cavity absorption or stimulated emission. A noteworthy feature is the persistence of bunching, although the bunching is less than that of chaotic light.